2016
DOI: 10.1016/j.nds.2016.02.001
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Nuclear Data Sheets for A = 41

Abstract: A b s t r a c t :A v a i l a b l e i n f o r m a t i o n p e r t a i n i n g t o t h e n u c l e a r s t r u c t u r e o f a l l n u c l e i w i t h m a s s n u m b e r s A = 4 1 ranging from Al (Z=13) to Ti (Z=22) are presented. The experimental reaction and decay data are evaluated and a n y i n c o n s i s t e n c i e s o r d i s c r e p a n c i e s a r e n o t e d . T h e a d o p t e d v a l u e s f o r v a r i o u s l e v e l p r o p e r t i e s ( s u c h a s t h e spin, parity and and halflife) and gamma… Show more

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Cited by 27 publications
(45 citation statements)
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“…For ν e,µ,τ + e − events, gamma rays can be produced through bremsstrahlung, but that is suppressed because the event energies are well below the critical energy of 32 MeV [45][46][47]. And for neu- tron capture, the total energy release is 6.1 MeV, with at most one gamma ray having substantial energy [72][73][74]. Further study is needed to assess the the potential to separate these event classes from each other (as well as from the less-important backgrounds due to ν e,µ,τ + 40 Ar events and spallation beta decays).…”
Section: B4 Particle-identification Techniquesmentioning
confidence: 99%
“…For ν e,µ,τ + e − events, gamma rays can be produced through bremsstrahlung, but that is suppressed because the event energies are well below the critical energy of 32 MeV [45][46][47]. And for neu- tron capture, the total energy release is 6.1 MeV, with at most one gamma ray having substantial energy [72][73][74]. Further study is needed to assess the the potential to separate these event classes from each other (as well as from the less-important backgrounds due to ν e,µ,τ + 40 Ar events and spallation beta decays).…”
Section: B4 Particle-identification Techniquesmentioning
confidence: 99%
“…This required that the activation happened in two steps with a cool down time in between. 41 Ar decays into stable 41 K with a half-life of 109.6 min [24]. Hence, its activity decreased below 1 Bq after 2 days and was negligible after ∼ 160 days when the source was introduced into the detector.…”
Section: Source Productionmentioning
confidence: 99%
“…(2) but are neglected by state of the art approaches. Note that there are more than 200 experimentally observed excitations already between the ground state and the neutron separation threshold in 41 Ca [49], while the SCGF-ADC(3) predicts only about 40 of them. This issue is likely to worsen at higher energies where configurations more complex than 2p1h become relevant.…”
mentioning
confidence: 99%